期刊
ASTROPHYSICAL JOURNAL
卷 562, 期 2, 页码 L129-L132出版社
IOP PUBLISHING LTD
DOI: 10.1086/338325
关键词
conduction; cooling flows; galaxies : clusters : general; magnetic fields
We estimate the thermal conductivity of a weakly collisional magnetized plasma with chaotic magnetic field fluctuations. When the fluctuation spectrum extends over two or more decades in wavevector, we find that thermal conduction is very efficient; the conduction coefficient is only a factor of similar to5 below the classical Spitzer estimate. We suggest that conduction could play a significant role in cooling flows in clusters of galaxies.
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